Konstantin Ladutenko 7 years ago
parent
commit
022ade84d4
1 changed files with 38 additions and 28 deletions
  1. 38 28
      main.tex

+ 38 - 28
main.tex

@@ -423,14 +423,15 @@ length will be around 5--10~nm for $N_e$ close to $N_{cr}$.
 \centering
 \centering
 \includegraphics[width=0.495\textwidth]{mie-fdtd-3}
 \includegraphics[width=0.495\textwidth]{mie-fdtd-3}
 \caption{\label{mie-fdtd} (a, b) First four Lorentz-Mie coefficients
 \caption{\label{mie-fdtd} (a, b) First four Lorentz-Mie coefficients
-  ($a_1$, $a_2$, $b_1$, $b_2$) and factors of asymmetry $G_I$, $G_{I^2}$ 
-  according to Mie theory at fixed wavelength $800$~nm. (c, d) Intensity
-  distribution calculated by Mie theory and (e, f) EHP distribution
-  for low free carrier densities $N_e \approx 10^{20}$~cm$^{-3}$ by
-  Maxwell's equations (\ref{Maxwell}, \ref{Drude}) coupled with EHP
-  density equation (\ref{Dens}). (c-f) Incident light propagates from
-  the left to the right along $Z$ axis, electric field polarization
-  $\vec{E}$ is along $X$ axis.}
+  ($a_1$, $a_2$, $b_1$, $b_2$) and factors of asymmetry $G_I$,
+  $G_{I^2}$ according to Mie theory at fixed wavelength $800$~nm. (c,
+  d) Squared intensity distribution calculated by Mie theory and (e,
+  f) EHP distribution for low free carrier densities
+  $N_e \approx 10^{20}$~cm$^{-3}$ by Maxwell's equations
+  (\ref{Maxwell}, \ref{Drude}) coupled with EHP density equation
+  (\ref{Dens}). (c-f) Incident light propagates from the left to the
+  right along $Z$ axis, electric field polarization $\vec{E}$ is along
+  $X$ axis.}
 \end{figure}
 \end{figure}
 
 
 The changes of the real and imaginary parts of the permittivity
 The changes of the real and imaginary parts of the permittivity
@@ -486,15 +487,22 @@ license.
 
 
 %\subsection{Effect of the irradiation intensity on EHP generation}
 %\subsection{Effect of the irradiation intensity on EHP generation}
 
 
- Firstly, we analyze Mie coefficients (Fig.~\ref{mie-fdtd}) and the
- intensity distribution inside the non-excited Si NP as a function of
- its size for a fixed laser wavelength $\lambda = 800$~nm.  We
- introduce $G_I$ factor of asymmetry, corresponding to difference
- between the volume integral of intensity in the front side of the NP
- to that in the back side normalized to their sum:
+ We start with a pure electromagnetic problem without EHP
+ generation. We plot in Fig.~\ref{mie-fdtd}(a) Mie coefficients of a
+ Si NP as a function of its size for a fixed laser wavelength
+ $\lambda = 800$~nm.  For the NP sizes under consideration most of
+ contribution to the electromagnetic response originates from electric
+ and magnetic dipole (ED and MD), while for sizes near
+ $R \approx 150$~nm a magnetic quadrupole (MQ) response turns to be
+ the main one. The superposition of multipoles defines the
+ distribution of electric field inside of the NP.  We introduce $G_I$
+ factor of asymmetry, corresponding to difference between the volume
+ integral of intensity in the front side of the NP to that in the back
+ side normalized to their sum:
  $G_I = (I^{front}-I^{back})/(I^{front}+I^{back})$, where
  $G_I = (I^{front}-I^{back})/(I^{front}+I^{back})$, where
  $I^{front}=\int_{(z>0)}|E|^2d{\mathrm{v}}$ and
  $I^{front}=\int_{(z>0)}|E|^2d{\mathrm{v}}$ and
- $I^{back}=\int_{(z<0)} |E|^2d{\mathrm{v}}$. The factor $G_{I^2}$ was
+ $I^{back}=\int_{(z<0)} |E|^2d{\mathrm{v}}$ are expressed via
+ amplitude of the electric field $|E|$. The factor $G_{I^2}$ was
  determined in a similar way by using volume integrals of squared
  determined in a similar way by using volume integrals of squared
  intensity to predict EHP asymmetry due to two-photon absorption.
  intensity to predict EHP asymmetry due to two-photon absorption.
  Fig.~\ref{mie-fdtd}(b) shows $G$ factors as a function of the NP
  Fig.~\ref{mie-fdtd}(b) shows $G$ factors as a function of the NP
@@ -506,26 +514,28 @@ license.
  side of the NP as demonstrated in Fig.~\ref{mie-fdtd}(d). In fact,
  side of the NP as demonstrated in Fig.~\ref{mie-fdtd}(d). In fact,
  very similar EHP distributions can be obtained by applying Maxwell's
  very similar EHP distributions can be obtained by applying Maxwell's
  equations coupled with the rate equation for relatively weak
  equations coupled with the rate equation for relatively weak
- excitation $N_e \approx 10^{20}$~cm$^{-3}$. The optical properties do
- not change considerably due to the excitation according to
- (\ref{Index}). Therefore, the excitation processes follow the
- intensity distribution. However, such coincidence was achieved under
- quasi-stationary conditions, after the electric field made enough
- oscillations inside the Si NP.
- 
- To achieve a qualitative description of the EHP distribution, we
- introduced another asymmetry factor
+ excitation with EHP concentration of $N_e \approx
+ 10^{20}$~cm$^{-3}$. The optical properties do not change considerably
+ due to the excitation according to (\ref{Index}). Therefore, the
+ excitation processes follow the intensity distribution. However, such
+ coincidence was achieved under quasi-stationary conditions, after the
+ electric field made enough oscillations inside the Si NP, transient
+ analysis reveal much more details.
+
+ To achieve a qualitative description for evolution of the EHP
+ distribution during the \textit{fs} pulse, we introduced another
+ asymmetry factor
  $G_{N_e} = (N_e^{front}-N_e^{back})/(N_e^{front}+N_e^{back})$
  $G_{N_e} = (N_e^{front}-N_e^{back})/(N_e^{front}+N_e^{back})$
  indicating the relationship between the average EHP densities in the
  indicating the relationship between the average EHP densities in the
- front and in the back parts of the NP. This way, $G_{N_e} = 0$
+ front and in the back halfs of the NP. This way, $G_{N_e} = 0$
  corresponds to the quasi-homogeneous case and the assumption of the
  corresponds to the quasi-homogeneous case and the assumption of the
  NP homogeneous EHP distribution can be made to investigate the
  NP homogeneous EHP distribution can be made to investigate the
  optical response of the excited Si NP. When $G_{N_e}$ significantly
  optical response of the excited Si NP. When $G_{N_e}$ significantly
  differs from $0$, this assumption, however, could not be
  differs from $0$, this assumption, however, could not be
  justified. In what follows, we discuss the results of the numerical
  justified. In what follows, we discuss the results of the numerical
- modeling revealing the EHP evolution stages during pulse duration
- shown in Fig.~\ref{plasma-grid} and the temporal/EHP dependent evolution of
- the asymmetry factor $G_{N_e}$ in Fig.~\ref{time-evolution}.
+ modeling of the temporal evolution of the asymmetry factor $G_{N_e}$
+ in Fig.~\ref{time-evolution} revealing the EHP evolution stages during pulse
+ duration shown in Fig.~\ref{plasma-grid}.
 
 
  % Fig. \ref{Mie} demonstrates the temporal evolution of the EHP
  % Fig. \ref{Mie} demonstrates the temporal evolution of the EHP
  % generated inside the silicon NP of $R \approx 105$~nm. Here,
  % generated inside the silicon NP of $R \approx 105$~nm. Here,